# File:StabilityDiagramsIdaItokawa.png

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Stability diagram around Ida (left panel) and around Itokawa (right panel): the chaotic domain is shown by the reddish area. Chaos is determined by computing the Lyapunov exponent $$\Lambda$$ for a trajectory with initial orbital elements $$(q, e)$$. On Left panel, the black dot marks the dynamical locus of Dactyl, moon of Ida(from Lages J., Shepelyansky D.L., Shevchenko I.I. (2017). Chaotic zones around rotating small bodies, Astronomical Jour. 153, 272)

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Date/Time Thumbnail Dimensions User Comment current 18:32, 15 August 2017 1,024 × 483 (1.4 MB) José Lages (Talk | contribs) Stability diagram around Ida (left panel) and around Itokawa (right panel): the chaotic domain is shown by the reddish area. Chaos is determined by computing the Lyapunov exponent $$\Lambda$$ for a trajectory with initial orbital elements $$(q, e)$$. O...

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